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Application of Convolutional Neural Networks to Identify Stellar Feedback Bubbles in CO Emission

  • Authors: Duo Xu, Stella S.R. Offner, Robert Gutermuth, and Colin Van Oort

2020 The Astrophysical Journal 890 64.

  • Provider: AAS Journals

Caption: Figure 2.

Upper row: 13CO integrated intensity including emission from the full cloud. Bottom row: integrated intensity of the full 13CO (upper row) masked by a 13CO synthetic observation of the tracer field to obtain the pixel locations of the feedback in PPV space (see Section 2.3.2). First column: synthetic observations corresponding to model W2_T2_t0 in Offner & Arce (2015). Second column: synthetic observations corresponding to model W2_T2_t1. Third column: synthetic observations corresponding to model W1_T2_t0. Fourth column: synthetic observations corresponding to model W2_T3_t0.

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